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20242026
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astro-ph.SR2026

Unveiling Complex Chemistry in Planet-forming Disks with the SKAO

Linda Podio, Lisa Giani, Catherine Walsh +38

The chemical composition of planets is inherited from that of the natal protoplanetary disk at the time of planet formation. In recent years, we have made huge progress in characte…

astro-ph.SR2026

Astrochemical Study of Early Embedded Disks

Eleonora Bianchi

The question of how our planet was formed and, more generally, how a planetary system forms is fundamental and has been addressed in a broad range of research domains. However, we…

astro-ph.SR2026

Chemical Complexity in the Early Stages of Star Formation in the SKAO Era

Eleonora Bianchi, Mathilde Bouvier, Claudio Codella +44

About 350 molecules have been identified in the interstellar medium (ISM), including complex molecules relevant to prebiotic chemistry. A remarkable level of molecular diversity ha…

astro-ph.SR2026

FAUST XXXI. Grain properties and variability of three sources in GSS 30

Q. Yang, H. Baobab Liu, S. Feng +55

To advance our understanding of dust properties in class 0/I young stellar objects, it is crucial to resolve their structures at multiple wavelengths and investigate how grain grow…

astro-ph.SR2026

High-resolution mid-IR spectroscopy of SVS 13-A with EXES/SOFIA: The surprisingly high CHOH/HO ratio in the planet-forming zone of a solar mass protostar

Curtis DeWitt, Marta De Simone, Eleonora Bianchi +8

Water and methanol are key components of interstellar ices and gas in star- and planet-forming regions, but direct observations of water in low-mass protostars are challenging due…

astro-ph.SR2025

FAUST. XXVIII. High-Resolution ALMA Observations of Class 0/I Disks: Structure, Optical Depths, and Temperatures

M. J. Maureira, J. E. Pineda, H. B. Liu +22

We present high-resolution (~7.5 au) ALMA observations at 1.3 and 3 mm of 16 disks around Class 0/I protostars across multiple star-forming regions and a variety of multiplicities,…